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| Journal Article | PUBDB-2022-04150 |
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2022
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Please use a persistent id in citations: doi:10.1007/JHEP07(2022)084 doi:10.3204/PUBDB-2022-04150
Report No.: DESY-21-172; ULB-TH/21-17; arXiv:2110.13926
Abstract: Dark Matter could be a composite state of a confining sector with an approximate scale symmetry. We consider the case where the associated pseudo-Goldstone boson, the dilaton, mediates its interactions with the Standard Model. When the confining phase transition in the early universe is supercooled, its dynamics allows for Dark Matter masses up to 10$^{6}$ TeV. We derive the precise parameter space compatible with all experimental constraints, finding that this scenario can be tested partly by telescopes and entirely by gravitational waves.
Keyword(s): critical phenomena: confinement ; dark matter: mass ; dark matter: composite ; up: mass ; dilaton ; gravitational radiation ; mediation ; Goldstone particle ; Beyond Standard Model ; Confinement ; Cosmology of Theories beyond the SM ; Technicolor and Composite Models
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Preprint
Supercool Composite Dark Matter beyond 100 TeV
[10.3204/PUBDB-2021-04197]
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